1986
DOI: 10.1007/bf00474112
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A century of spectral interferences in atomic emission spectroscopy — Can we master them with modern apparatus and approaches?

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Cited by 55 publications
(7 citation statements)
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“…Spectral interferences, especially line overlaps, can be a major problem in ICP-AES. [35][36][37] Although efforts have been made to collect spectral interference data in different matrices [38][39][40][41] or to build in databases in commercial ICP-AES instruments to help users select emission lines free from spectral interference in different matrices, 42 the selection of an appropriate analytical line can still be difficult, especially for a sample with a complex or unknown matrix. Improper line selection results in a loss of detection power and analytical errors.…”
Section: Spectral Interference By Matrixmentioning
confidence: 99%
“…Spectral interferences, especially line overlaps, can be a major problem in ICP-AES. [35][36][37] Although efforts have been made to collect spectral interference data in different matrices [38][39][40][41] or to build in databases in commercial ICP-AES instruments to help users select emission lines free from spectral interference in different matrices, 42 the selection of an appropriate analytical line can still be difficult, especially for a sample with a complex or unknown matrix. Improper line selection results in a loss of detection power and analytical errors.…”
Section: Spectral Interference By Matrixmentioning
confidence: 99%
“…Spectral interferences are the most severe problems in the elaboration of ICP-AES methods [37][38][39][40][41]. The actual number of lines emitted from an ICP excitation source is much higher than the number of spectral lines listed in the classical tables [42,43].…”
Section: Spectral Interferences and Line Selectionmentioning
confidence: 99%
“…Although robust, this design is sensitive to interferences caused by strong spectral components -both from those that are directly detected and from those that fall outside the field-of-view and lights up the otherwise completely dark interior. This undesired light is usually referred to as stray light [7][8][9][10] and stems primary from scattering upon optics and dust as well as reflections on the inner walls. The error -manifested as an intensity offset -caused by stray light is often not significant in comparison to the intensity of a relatively intense spectral line, yet it leads to experimental difficulties monitoring weaker ones accurately.…”
Section: Introductionmentioning
confidence: 99%